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Extensions of the standard model that lead to first-order phase transitions in the early universe can produce a stochastic background of gravitational waves, which may be accessible to future detectors.
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E. Bennett, D.K. Hong, H. Hsiao, J.W. Lee, C.J.D. Lin, B. Lucini, M. Mesiti, M. Piai, D. Vadacchino, Phys. Rev. D 106
2022
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S. Kulkarni, A. Maas, S. Mee, M. Nikolic, J. Pradler, F. Zierler (2022), 2202.05191
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M. Reichert, Z.W. Wang, Gravitational Waves from dark composite dynamics (2022), 2211.08877
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